Take a flight over Korolev Crater on Mars

We love flyover videos from other worlds. These stunning videos, created from imagery gathered by orbiting spacecraft, can give us a sense of what it would be like to fly in an airplane on another planet. This latest flyover video from the European Space Agency’s Mars Express spacecraft, provides a stunning view of one of Mars’ most eye-popping craters.

This movie was created using an imagery from Mars Express’ High Resolution Stereo Camera (HRSC).  The images are normally taken looking straight down (nadir), and the video combines topography information from the stereo channels of HRSC to generate a three-dimensional landscape, which was then recorded from different perspectives, as with a movie camera, to render the flight shown in the video.

Korolev Crater is 82 kilometers (50 miles) across and at least 2 km (1.25 miles) deep. This well-preserved crater is located the northern lowlands of Mars, just south of a large patch of dune-filled terrain that encircles part of the planet’s northern polar cap (known as Olympia Undae).

Overhead view of Korolev Crater on Mars, as seen by the European Space Agency’s Mars Express spacecraft.Overhead view of Korolev Crater on Mars, as seen by the European Space Agency’s Mars Express spacecraft.

That’s not snow you’re seeing, but this crater is constantly filled with water ice, and its central mound is about 1.8 kilometers (1.1 miles) thick all year round. It’s one of the largest reservoirs of non-polar ice on Mars.

This view reminds me of a flight I took where I flew over Meteor Crater in Arizona USA. But for comparison, Meteor Crater is less than a mile across (.737 miles/1.186 km) and just 560 feet (170 m) deep.

The view of Meteor Crater from an airplane during a cross-country commercial flight.The view of Meteor Crater from an airplane during a cross-country commercial flight.

You may be thinking, how can this ice remain stable in Korolev Crater; doesn’t water ice sublimate away in Mars thin atmosphere? Just like dry ice does here on Earth, water ice on Mars usually goes from solid to gas with the low atmospheric pressure. (Mars has approximately 8 millibars while on Earth the average, atmospheric pressure at sea level is 1013.25 millibars, or about 14.7 pounds per square inch.)

But temperature can influence ice stability as well. Water ice is permanently stable within the Korolev Crater because the deepest part of this depression acts as a natural cold trap. The scientists at ESA explain that the air above the ice cools and is thus heavier compared to the surrounding air: since air is a poor conductor of heat, the water ice mound is effectively shielded from heating and sublimation.

The name of the crater may be familiar. It’s named after Russian rocket engineer and spacecraft designer Sergei Pavlovich Korolev (1907-1966). He developed the first Russian intercontinental rocket R7, the precursor of the modern Soyuz rockets that are still operated today. With his rocket and spacecraft design, he was also responsible for the first human-made satellite (Sputnik in 1957) and for the first human spaceflight (Yuri Gagarin in 1961).

Find out more about Mars Express and Korolev Crater here and here.

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By Nancy Atkinson

Nancy has been with Universe Today since 2004. She is the author of a new book on the Apollo program, "Eight Years to the Moon," which shares the stories of 60 engineers and scientists who worked behind the scenes to make landing on the Moon possible. Her first book, "Incredible Stories from Space: A Behind-the-Scenes Look at the Missions Changing Our View of the Cosmos" tells the stories of those who work on NASA's robotic missions to explore the Solar System and beyond.

(Source: universetoday.com; July 3, 2020; https://tinyurl.com/ybhj2qxl)
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